Q87706637

Summary

Q87706637 is a rotating variable star^[1].

Key Facts

• Q87706637's instance of is recorded as rotating variable star^[2].
• Q87706637's instance of is recorded as star^[3].
• Q87706637's instance of is recorded as near-infrared source^[4].
• Q87706637's constellation is recorded as Lyra^[5].
• Q87706637's spectral class is recorded as G5V^[6].
• Q87706637's child astronomical body is recorded as Q28856021^[7].
• Q87706637's catalog code is recorded as Gaia DR2 2052653729346427136^[8].
• Q87706637's catalog code is recorded as KOI-1218^[9].
• Q87706637's catalog code is recorded as 2MASS J19240457+3832440^[10].
• Q87706637's catalog code is recorded as KIC 3442055^[11].
• Q87706637's catalog code is recorded as Kepler-795^[12].
• Q87706637's catalog code is recorded as Kepler-795A^[13].
• Q87706637's catalog code is recorded as Gaia DR3 2052653729346427136^[14].
• Q87706637's catalog code is recorded as TIC 122684233^[15].
• Q87706637's catalog code is recorded as SPOCS 3335^[16].
• Q87706637's type of variable star is recorded as rotating variable star^[17].
• Q87706637's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.143'}^[18].
• Q87706637's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.708'}^[19].
• Q87706637's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.77'}^[20].
• Q87706637's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.298518'}^[21].
• Q87706637's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.42'}^[22].
• Q87706637's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.8927124'}^[23].
• Q87706637's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.989'}^[24].
• Q87706637's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.0378'}^[25].
• Q87706637's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0228'}^[26].

Body

Definition and Type

Recorded instance of include rotating variable star^[2], star^[3], and near-infrared source^[4].